The central heart was of crimson-colored natives; the one to the right of pale orange, and the left of bright blue. It was ten seconds in forming, and five seconds in dispersing. The number engaged in the evolution could not be less than half a million.

Thus has been solved one of the great astronomical questions of the century.

The next evening the committee assembled earlier, so as to get a view of the planet Venus before the moon rose. It was the first time that the lad's attention had been drawn to any of the planets, and he evinced the liveliest joy when he first beheld the cloudless disk of that resplendent world. It may here be stated that his power of vision, in looking at the fixed stars, was no greater or less than that of an ordinary eye. They appeared only as points of light, too far removed into the infinite beyond to afford any information concerning their properties. But the committee were doomed to a greater disappointment when they inquired of the boy what he beheld on the surface of Venus. He replied, "Nothing clearly; all is confused and watery; I see nothing with distinctness." The solution of the difficulty was easily apprehended, and at once surmised. The focus of the eye was fixed by nature at 240,000 miles, and the least distance of Venus from the earth being 24,293,000 miles, it was, of course, impossible to observe that planet's surface with distinctness. Still she appeared greatly enlarged, covering about one hundredth part of the heavens, and blazing with unimaginable splendor.

Experiments upon Jupiter and Mars were equally futile, and the committee half sorrowfully turned again to the inspection of the moon.

The report then proceeds at great length to give full descriptions of the most noted geographical peculiarities of the lunar surface, and corrects many errors fallen into by Herschel, Leverrier and Proctor. Professor Secchi informs us that the surface of the moon is much better known to astronomers than the surface of the earth is to geographers; for there are two zones on the globe within the Arctic and Antarctic circles, that we can never examine. But every nook and cranny of the illuminated face of the moon has been fully delineated, examined and named, so that no object greater than sixty feet square exists but has been seen and photographed by means of Lord Rosse's telescope and De la Ruis' camera and apparatus. As the entire report will be ordered published at the next weekly meeting of the College, we refrain from further extracts, but now proceed to narrate the results of our own interviews with the boy.

It was on the evening of the 17th of February, 1876, that we ventured with rather a misgiving heart to approach Culp Hill, and the humble residence of a child destined, before the year is out, to become the most celebrated of living beings. We armed ourselves with a pound of sugar candy for the boy, some muslin-de-laine as a present to the mother, and a box of cigars for the father. We also took with us a very large-sized opera-glass, furnished for the purpose by M. Muller. At first we encountered a positive refusal; then, on exhibiting the cigars, a qualified negative; and finally, when the muslin and candy were drawn on the enemy, we were somewhat coldly invited in and proffered a seat. The boy was pale and restless, and his eyes without bandage or glasses. We soon ingratiated ourself into the good opinion of the whole party, and henceforth encountered no difficulty in pursuing our investigations. The moon being nearly full, we first of all verified the tests by the committee. These were all perfectly satisfactory and reliable. Requesting, then, to stay until after midnight, for the purpose of inspecting Mars with the opera-glass, we spent the interval in obtaining the history of the child, which we have given above.

The planet Mars being at this time almost in dead opposition to the sun, and with the earth in conjunction, is of course as near to the earth as he ever approaches, the distance being thirty-five millions of miles. He rises toward midnight, and is in the constellation Virgo, where he may be seen to the greatest possible advantage, being in perigee. Mars is most like the earth of all the planetary bodies. He revolves on his axis in a little over twenty-four hours, and his surface is pleasantly variegated with land and water, pretty much like our own world—the land, however, being in slight excess. He is, therefore, the most interesting of all the heavenly bodies to the inhabitants of the earth.

Having all things in readiness, we directed the glass to the planet. Alas, for all our calculations, the power was insufficient to clear away the obscurity resulting from imperfect vision and short focus.

Swallowing the bitter disappointment, we hastily made arrangements for another interview, with a telescope, and bade the family good night.

There is but one large telescope properly mounted in the city, and that is the property and pride of its accomplished owner, J. P. Manrow, Esq. We at once procured an interview with that gentleman, and it was agreed that on Saturday evening the boy should be conveyed to his residence, picturesquely situated on Russian Hill, commanding a magnificent view of the Golden Gate and the ocean beyond.